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Atmospheric Convection Plays a Key Role in the Climate of Tidally Locked Terrestrial Exoplanets: Insights from High-resolution Simulations

  • Authors: Denis E. Sergeev, F. Hugo Lambert, Nathan J. Mayne, Ian Boutle, James Manners, and Krisztian Kohary

2020 The Astrophysical Journal 894 84.

  • Provider: AAS Journals

Caption: Figure 2.

Surface temperature (shading, ﹩{\rm{K}}﹩) and horizontal wind vectors in the upper troposphere (﹩250\,\mathrm{hPa}﹩ level) in the (left column panels) Trappist-1e case and (right column) Proxima b case in (a) and (b) MassFlux, and (c)–(f) sensitivity simulations. The surface temperature in (c) and (d) Adjust, and (e) and (f) NoCnvPm simulations is shown as the difference relative to the MassFlux simulation.

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